Regional trends in European induction data     

Karel Pěč  Jana Pěčová  Oldřich Praus  Reviewer M. Hvoždara 《Studia Geophysica et Geodaetica》1977,21(3-4):383-393

n ¶rt;a, n¶rt;mau 531 au ¶rt; u aum m u¶rt;uu n mumu ana¶rt;, ¶rt; u -m n, aauum ¶rt;um u u amuaa n¶rt;naa ma ua aama. uu nmam an¶rt;u ¶rt; u aum aam ¶rt;au cuu uP _n ^m , n¶rt;am mn n=1, 2, 3 u 5 (m n). u uua ¶rt;a¶rt;amu uu n¶rt;mauu uum au (a. 1) u u n aumam uu nmu, m n¶rt;mam u¶rt; am uuu ¶rt; u aum (u. 1–4). annuau 2 u 5 mn nm ma am mmmu m (u. 5, 6). ama uuu u m aam amu uu uma.  相似文献   

Electromagnetic induction in a spherical earth with a circular bulge in the upper mantle     

Milan Hvoždara  Reviewer V. Petr 《Studia Geophysica et Geodaetica》1977,21(3-4):374-382

Summary Results of computing the anomalies of the variable magnetic field, generated by a harmonically variable field of the H_1,0-type in the model of a spherical Earth with an expressive bulge in the well-conducting part of the mantle, are presented. It was found that not only the radial, but also the tangential component of the magnetic field is disturbed above the bulge. The largest amplitudes of these changes can be observed over the area of the largest slope of the conductivity boundary if the exciting magnetic field is perpendicular to the surface of the interface.  相似文献   

Frequency limitation to the theoretical investigation of the transmission of hm waves through the ionosphere     

Josef Bochníček  Reviewer M. Hvoždara 《Studia Geophysica et Geodaetica》1974,18(4):405-408

Summary As a result of investigating the energy flow, transmitted by short-period HM waves, the existence of a frequency limitation was found at the theoretical investigation of the propagation of these HM waves.  相似文献   

New Definition of Discovery for Solar System Objects     

Andrea Milani  Giovanni F. Gronchi  Zoran Knežević 《Earth, Moon, and Planets》2007,100(1-2):83-116

We propose a new formal definition of discovery for a Solar System object. It is based on an objective and mathematically rigorous algorithm to assess when a set of observations is enough to constitute a discovery. When this definition is satisfied, in almost all cases the orbit is defined well enough to establish the nature of the object discovered (Main Belt vs. Near Earth Asteroid, Trans-Neptunian vs. long period comet). The frequency of occurrence of exceptions is estimated by a set of numerical experiments. The availability of a non-subjective definition of discovery allows some rules to be adopted for the assignment of discovery credit with a minimum risk of dispute. Such rules should be fair, encourage good practice by the observers and acknowledge the contribution of the orbit computers providing the identifications and the orbits, as well as the one of all the contributing observers.  相似文献   

Dynamical portrait of the Lixiaohua asteroid family     

B. Novaković  K. Tsiganis  Z. Knežević 《Celestial Mechanics and Dynamical Astronomy》2010,107(1-2):35-49

In this paper we present a comprehensive analysis of the dynamics in the region of the (3556) Lixiaohua asteroid family. The family lies in a particularly interesting region of the phase space, crossed by several two-body and three-body mean motion resonances. Also, members of this family can have close encounters with large asteroids, such as Ceres. We have identified the mean motion resonances which contribute to the long-term dynamical evolution of the family and our results confirm that the members of this family can be classified into a number of groups, exhibiting different dynamical behavior. We show for the first time that in the Lixiaohua region, apart from the chaotic diffusion in proper eccentricity and inclination (e _p and I _p ), there is at least one extended chaotic zone where several resonances overlap, thus giving rise to chaotic diffusion in proper semi-major axis (a _p ) as well. Using a code of Monte Carlo type, we simulate the evolution of the family, according to the model which combines the chaotic diffusion (in a _p , e _p and I _p ), Yarkovsky/YORP thermal effect and random walk in a _p due to the close encounters with massive asteroids. These simulations show that all these effects should be taken into account in order to accurately explain the observed distribution of family members in the space of proper elements, although a “minimal” model that accounts for chaotic diffusion in (e _p , I _p ), Yarkovsky-induced drift in a _p and random walk in a _p due to the close encounters with the most massive asteroids is enough to grossly characterize the shape of the family.  相似文献   

Modelling tidal current‐induced bed shear stress and palaeocirculation in an epicontinental seaway: the Bohemian Cretaceous Basin,Central Europe     

ANDREW J. MITCHELL  DAVID ULIČNÝ  GARY J. HAMPSON  PETER A. ALLISON  GERARD J. GORMAN  MATTHEW D. PIGGOTT  MARTIN R. WELLS  CHRISTOPHER C. PAIN 《Sedimentology》2010,57(2):359-388

Lower to Middle Turonian deposits within the Bohemian Cretaceous Basin (Central Europe) consist of coarse‐grained deltaic sandstones passing distally into fine‐grained offshore sediments. Dune‐scale cross‐beds superimposed on delta‐front clinoforms indicate a vigorous basinal palaeocirculation capable of transporting coarse‐grained sand across the entire depth range of the clinoforms (ca 35 m). Bi‐directional, alongshore‐oriented, trough cross‐set axes, silt drapes and reactivation surfaces indicate tidal activity. However, the Bohemian Cretaceous Basin at this time was over a thousand kilometres from the shelf break and separated from the open ocean by a series of small islands. The presence of tidally‐influenced deposits in a setting where co‐oscillating tides are likely to have been damped down by seabed friction and blocked by emergent land masses is problematic. The Imperial College Ocean Model, a fully hydrodynamic, unstructured mesh finite element model, is used to test the hypothesis that tidal circulation in this isolated region was capable of generating the observed grain‐size distributions, bedform types and palaeocurrent orientations. The model is first validated for the prediction of bed shear stress magnitudes and sediment transport pathways against the present‐day North European shelf seas that surround the British Isles. The model predicts a microtidal to mesotidal regime for the Bohemian Cretaceous Basin across a range of sensitivity tests with elevated tidal ranges in local embayments. Funnelling associated with straits increases tidal current velocities, generating bed shear stresses that were capable of forming the sedimentary structures observed in the field. The model also predicts instantaneous bi‐directional currents with orientations comparable with those measured in the field. Overall, the Imperial College Ocean Model predicts a vigorous tide‐driven palaeocirculation within the Bohemian Cretaceous Basin that would indisputably have influenced sediment dispersal and facies distributions. Palaeocurrent vectors and sediment transport pathways however vary markedly in the different sensitivity tests. Accurate modelling of these parameters, in this instance, requires greater palaeogeographic certainty than can be extracted from the available rock record.  相似文献   

2D geological–geophysical model of the Timok Complex (Serbia,SE Europe): a new perspective from aeromagnetic and gravity data     

Snežana Ignjatović  Ivana Vasiljević  Milenko Burazer  Miodrag Banješević  Ivan Strmbanović  Vladica Cvetković 《Swiss Journal of Geoscience》2014,107(1):101-112

The study reports new aeromagnetic and gravity data for the northern part of the Timok Magmatic Complex (TMC), East Serbia. The TMC is part of the Tethyan Eurasian metallogenic zone well known for hosting large copper and gold deposits. The complex formed by continuous volcanic activity 90–78 Ma ago, that developed in roughly three phases: Turonian andesites, Santonian–Campanian andesites/basaltic andesites (both mostly volcanic) and Campanian latites/monzonites (mostly shallow intrusive). The aeromagnetic measurements included acquiring total magnetic intensity data that were corrected for diurnal variations, leveling, microleveling, calculated normal field values, calculated anomaly values of total magnetic field intensity and reduction to the pole. The gravity measurements were carried out in an irregular grid with relative gravity values obtained using a Worden gravity meter. 2D modeling reveals that the subsurface extension of the Campanian Valja Str? pluton is ten times larger than it is indicated by its surface outcrops. This implies that the area south and southeast from the pluton can be interesting in terms of finding new porphyry systems. The model indicates that this intrusive body should not be considered as a deeply dissected pluton. This sheds new light onto its potential with respect to epithermal gold mineralization, as well. The model also suggests that there are larger non-exposed bodies of Santonian–Campanian volcanics and near-surface hydrothermally altered rocks than it is inferred from geological maps. The results of our study suggest that further interdisciplinary investigations in the TMC, in particular those integrating geophysics and geology, may have potential of advancing the existing exploration models.  相似文献   

Forcing mechanisms of a heavy precipitation event in the southeastern Adriatic area     

Branka Ivančan-Picek  Kristian Horvath  Nataša Strelec Mahović  Marjana Gajić-Čapka 《Natural Hazards》2014,72(2):1231-1252

The aim of this study was to identify the main mesoscale features and mechanisms responsible for the generation of an extreme precipitation event as a contribution to improving the modelling of processes that produce HPEs. The event occurred during the morning hours on 22 November 2010 over the Dubrovnik coast in Croatia and the hinterland mountain range of the southern Dinaric Alps and caused severe flash floods and landslides and consequent interruption of traffic and electricity supply as well as other infrastructural damage. The analysis is geographically focused on the southern portion of the eastern Adriatic region, which is prone to relatively frequent heavy precipitation events that occur mostly in autumn. This area is one of the rainiest in Europe with expected annual amounts of precipitation greater than 5,000 mm in the mountainous hinterland. The mechanisms responsible for the formation of convection were analysed using synop measurements, satellite data and numerical experiments performed with the WRF model, which was set up at the convection-permitting resolution in the innermost domain. Satellite data were used to identify the precipitation systems and to estimate the intensity of the precipitation during the period of interest. The development of the precipitation system was connected to a strong large-scale ascent over the southern Italy and southern Adriatic due to the advection of warm air and cyclonic vorticity advection, which increases with height. The numerical simulations highlighted the essential role of a southerly low-level jet stream in the transport of warm and moist air towards the affected area. The convergence of two branches of low-level marine air favoured convection triggered over the coast and sea. Furthermore, numerical sensitivity experiments suggested that the orography of the Dinaric Alps plays an essential role in the precipitation maximum over the mountainous hinterland, but also that the orography was not the crucial factor in the heavy precipitation near Dubrovnik. This study highlights the need for a dense network of observations, especially radar measurements, to validate the simulated mechanisms and improve numerical forecasts via data assimilation.  相似文献   

Direct detection of the secondary spectrum of the interacting eclipsing binary TX UMa     

J. Grygar  L. Hřič  R. Komžík  Z. Šíma 《Astrophysics and Space Science》1991,185(2):189-193

Eclipsing binary TX UMa was observed with the D.A.O. high-dispersion spectrographs in 1969–1970, with emphasis on the detailed coverage of the primary minimum. One spectrum was taken exclusively within totality, thus exhibiting an uncontaminated spectrum of the secondary component. This leads to spectral reclassification of the secondary (F6 IV). The narrowing of the line profile of the H-line in totality is interpreted in terms of synchronous rotation of the secondary (v sini80 km s^–1) while the primary rotates faster (v sini130 km s^–1) than synchronously (v sini50 km s^–1). Although the secondary does not fill in its Roche lobe fully, the system exhibits pronounced indications of rather strong physical interaction. This is now supported also by the profound changes of the line profiles of the H-line with phase.  相似文献   

Compositional variations in ferrotapiolite + tantalite pairs from the beryl-columbite pegmatite at Moravanynad Váhom, Slovakia     

M. Novák  P. Uher  P. Černý  P. Siman 《Mineralogy and Petrology》2000,69(3-4):295-306

Summary ?Three texturally and compositionally distinct pairs of ferrotapiolite + tantalite, all spatially related to a cleavelandite unit, were distinguished in the zoned beryl-columbite pegmatite at Moravany nad Váhom, Považsky Inovec Mts., Slovakia. (1) Inclusions of ferrotapiolite I (∼200 μm) in zoned ferrotantalite I exhibit crosscutting tielines of coexisting compositions in the columbite-tantalite quadrilateral. (2) Large ferrotapiolite II grains and adjacent, compositionaly variable grains of ferro- to manganotantalite II (∼100 μm) display remarkably diverse tielines, not yet observed in a single sample or locality. (3) Sn-depleted and slightly Mn,Ta-enriched narrow rims (∼20 μm) of ferrotapiolite III with small inclusions of manganotantalite III (≤ 5 μm) are located along a late, hydrothermal, fracture-filling microlite vein cross-cutting ferrotapiolite II. Changes in fO₂ derived from calculated Fe₂O₃ as well as variations in Ti, Sn, W concentrations through the ferrotapiolite + tantalite pairs I to III are negligible. Consequently, it seems plausible to explain the broadening of the two-phase field and the enrichment of ferrotapiolite and tantalite in Mn and Ta particularly by decreasing temperature. A disequilibrium crystallization from highly evolved residual melt and/or fluids is suggested for all textural types.

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Zusammenfassung ?Zusammensetzung von Ferrotapiolit-Tantalit-Paaren im Beryll-Columbit Pegmatit von Moravany nad Váhom (Považsky Inovec Mts., Slowakei) Drei Ferrotapiolit-Tantalit-Paare k?nnen in dem zonierten Beryll-Columbit-Pagmatit von Moravany nad Váhom, Povazsky Inovec Mts., Slowakei, auf der Basis detaillierter textureller und chemischer Untersuchungen unterschieden werden. Sie wurden in verschiedenen Stadien der Pegmatit-Kristallisation gebildet und sind r?mlich in Beziehung zu der Cleavelandit-Einheit (1). Einschlüsse von Ferrotapiolit I (∼200 μm) in zoniertem Ferrotantalit I zeigen sich kreuzende Konoden im Columbit-Tantalit Quadrilateral, die koexistierende K?rner beider Minerale miteinander verbinden. Dies legt nahe, dass Ferrotapiolit ein Produkt prim?rer (magmatischer) Disequilibrium-Kristallisation ist, und gleichzeitig mit den assoziierten Mineralen der Columbit-Gruppe gebildet wurde (2). Gro?e Ferrotapiolit II K?rner und K?rner von angrenzenden Ferro- bis Manganotantalit II (∼100 μm) zeigen Konoden mit bemerkenswerter Verschiedenheit, die bisher nicht in einer einzigen Probe beobachtet wurden. Eine sehr betonte Disequilibrium-Kristallisation aus stark fraktionierter Restschmelze dürfte hierfür verantwortlich sein (3). An Zinn verarmte und etwas an Mn, Ta angereicherter Ferrotapiolit III bildet dünne R?nder (∼20 μm) mit schmalen Einschlüssen von Manganotantalit III (≤5 μm) l?ngs einer Mikrolit-Ader. Erhat sich w?hrend hydrothermaler Subsolidus Verdr?ngung von Ferrotapiolit II durch Sprünge füllenden Microlit gebildet. Schwankungen in fO₂, berechnet aus Fe₂O₃ und die Gehalten an Ti, Sn und W k?nnen in den Ferrotapiolit-Tantalit-Paaren (1) bis (3) vernachl?ssigt werden. Dementsprechend erscheint es naheliegend, die Erweiterung des Zweiphasenfeldes und die Anreicherung von Ferrotapiolit und Tantalit an Mn und Ta durch Temperaturabnahme zu erkl?ren.

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Received May 4, 1999;/revised version accepted January 5, 2000  相似文献